Numerical simulation data for submission to Geophysical Research Letters: 'Flow Channels and the Generation of Alfvénic Turbulence along Storm-time Inner Magnetospheric Field-lines', C. C. Chaston 2022

Contains data from 3-D numerical simulation of inner magnetospheric flow channels:

1. 2-D data including the stream function, vector potential and normalized density from an equatorial slice through the 3-D simulation volume as a function of time.

2. 3-D data of the normalized density variation within the simulation volume.

3. Time arrays corresponding to the data above

All variables and spatial grids are defined in the manuscript under review from September 2022 with Geophysical Research Letters.